INGERSON LECTURE The composition of the continental crust*
Transcription
INGERSON LECTURE The composition of the continental crust*
Geochimicaet CosmochimicaActa, Vol. 59, No. 7, pp. 1217-1232, 1995 Copyright © 1995 ElsevierScienceLtd Printed in the USA. All rights reserved 0016-7037/95 $9.50 + .00 Pergamon 0016-7037(95)00038-0 INGERSON LECTURE The composition of the continental crust* K. HANS WEDEPOHL Geochemisches Institut, D-37077 G6ttingen, Germany A b s t r a c t - - A new calculation of the crustal composition is based on the proportions of upper crust ( U C ) to felsic lower crust ( F L C ) to mafic lower crust ( M L C ) of about 1:0.6:0.4. These proportions are derived from a 3000 km long refraction seismic profile through western Europe ( E G T ) comprising 60% old shield and 40% younger fold belt area with about 40 km average Moho depth. A granodioritic bulk composition of the UC in major elements and thirty-two minor and trace elements was calculated from the Canadian Shield data (Shaw et al., 1967, 1976). The computed abundance of thirty-three additional trace elements in the UC is based on the following proportions of major rock units derived from mapping: 14% sedimentary rocks, 25% granites, 20% granodiorites, 5% tonalites, 6% gabbros, and 30% gneisses and mica schists. The composition of FLC and MLC in major and thirty-six minor and trace elements is calculated from data on felsic granulite terrains and mafic xenoliths, respectively, compiled by Rudnick and Presper (1990). More than thirty additional trace element abundances in FLC and MLC were computed or estimated from literature data. The bulk continental crust has a tonalitic and not a dioritic composition with distinctly higher concentrations of incompatible elements including the heat producing isotopes in our calculation. A dioritic bulk crust was suggested by Taylor and McLennan ( 1985 ). The amount of tonalite in the crust requires partial melting of mafic rocks with about 100 km thickness (compared with about 7 km in the present M L C ) and water supply from dehydrated slabs and mafic intrusions. At the relatively low temperatures of old crustal segments M L C was partly converted into eclogite which could be recycled into the upper mantle under favourable tectonic conditions. The chemical fractionation of UC against FLC + M L C was caused by granitoidal partial melts and by mantle degassing which has controlled weathering and accumulation of volatile compounds close to the Earth's surface. FORMER ESTIMATES OF CRUSTAL COMPOSITION; SEISMIC CRUSTAL MODEL the geometry of the crust. EGT was long and variable enough to be representative of a typical crustal section. It comprises the Archean and Proterozoic Fennoscandian Shield with 45.5 km average Moho depth, the Late Proterozoic and Phanerozoic fold belts of Central Europe with 30 km crustal thickness, and the young Alpine orogen with its deep roots from the collision of two continents. The proportion of 60% old shield and 40% younger fold belts is representative of the state of the continental crust in different continents. A combination of the two crustal sections of different age gives an average crustal thickness of 40 km. A traveltime interpretation of the seismic refraction profile through the Fennoscandian Shield ( F E N N O L O R A ) , the transition from the Svecofennian Province in the Sorgenfrei-Tornquist Zone to the Danish and North German Basins ( E U G E N O S) and the younger fold belts in Central Europe ( E U G E M I and EGT-S 86) is presented in Fig. 1. At the right edge of the lower part of this cross section, Proterozoic and Phanerozoic Central Europe merges into the deep Alpine orogen in which the European and African crusts collided. For better presentation the simplified profile was divided into two parts. In Fig. 1 the continental crust consists of two major layers. The upper and lower crust can be conventionally separated according to P-wave velocities of less and more than 6.5 km/s. The interface occurs at almost 20 km depth in the upper part of Fig. 1 and is more variable in depth ( 2 0 - 5 0 km) in the The general acceptance of the definition of the continental crust as the continental upper part of the silicate Earth above the Mohorovici~ discontinuity dates back to the fifties of this century ( Poldervaart, 1955 ). Earlier authors as Clarke (1924) and Goldschmidt (1933) reported average chemical compositions of magmatic rocks or of what the latter author called the "lithosphere." Both averages were restricted to major units of the upper continental crust of our present definition. In this investigation we conclude from seismic properties on the thickness of the continental crust and the size and compositional characteristics of its major units. During the recent one and a half decade, refraction seismic ray velocities have been evaluated on a 4800 km long almost continuous traverse through Europe from the North Cape to Tunisia of which we used --3000 km (Ansorge et al., 1992). The European Geotraverse ( E G T ) was designed to encompass the succession of tectonic provinces from the oldest known Archean to those still active today. The tectonic provinces occur in succession from the north to the south as well as in time. The first step in understanding how the continental lithosphere of Europe formed was a survey of physical properties (density, etc.) in * Ingerson Lecture presented during the Goldschmidt Conference in Edinburgh, Scot August 31, 1994. The lecture was sponsored by the International Association of Geochemistry and Cosmochemistry. 1217 1218 K.H. Wedepohl Archean Crustal Province Scandinavian Caledonides, [ - - N ~ Barents Sea 0 Depth- Svecofennian Crustal Province 2040(km) 60- I 200 I 400 Sorgenfrei-Tornquist Zone, Baltic Sea I 600 I 800 I 1200 I 1000 Variscian Province North German Basin I 1400 km Alps ~~ 0Depth 2O 4O (km) :::!i:~i~::i~ii~iii~iiit::Ii:: ii~::iii::i::iiiiii i!iiii!iiiiiiiiiii~ ~ 1600 ~ 1800 Lithospheric Mantle (Vp > 6.1 km/s) 2000 2200 Mafic Granulites (Vp 6.9 - 7.5 km/s) 2400 2600 I 2800 km Sediments, Granites, Gneisses Felsic Granulites (Vp 6.5 - 6.9 km/s) (Vp < 6 - 6.5 km/s) FIG. 1. Simplified cross section of the crustal structure of the Baltic Shield and central Europe based on refraction seismic P-velocities derived from Figs. 3-4, 3-6, 3-9 and 3-11 in Ansorge et al. (1992) and from the detailed interpretations of FENNOLORA, EUGENO-S (Line 1), EUGEMI and EGT-S86 by Guggisberg et al. (1991), Aichroth et al. (1992), and Ye (1992). younger provinces presented in Fig. 1 (lower part). Superimposed on this basically two-layered crust are substantial lateral variations of the velocity distribution and layer thickness. Details in the uppermost crust of the Scandinavian profile are questionable because of large distances between the shotpoints in that part of the EGT. The major rocks below the interface at 20 km average depth and above the M o h o have been identified as granulites (for correlation of seismic properties with rock species see Kern and Schenk, 1988; Kern, 1990; Rudnick, 1992). The identification of major crustal rocks in the E U G E M I part of E G T was improved by the investigation of crustal xenoliths in the Tertiary volcanic rocks (Mengel et al., 1991 ). Luosto et al. ( 1 9 8 9 ) observed that the lower crust of the Scandinavian Shield is separated into a felsic upper part and a mafic lower part (the latter with more than 6.8 k m s i P-wave velocity) at an additional interface. Mafic granulites mainly from former gabbroic intrusions are recognized as the most abundant rocks in this lowest crustal layer of 7 k m average thickness. Confirmation of this identification as mafic granulites comes from areas of the world where these are sampled by volcanism and investigated as xenoliths (Rudnick 1992). Rare metapelitic garnet schists cannot be discriminated from the abundant mafic granulites by their seismic velocities (Kern, 1990). In the younger fold belts of Central Europe, mafic granulites occur locally as a voluminous body but more as a thin layer above the Moho. Because of difficulties to find out the thickness of the sedimentary top layer of the E G T crust we have used the estimate by Ronov and Yaroshevskiy ( 1 9 6 8 ) of a 2.9 k m thick unit of sedimentary rocks in the continental crust. This was based on drilling and mapping. In the young fold belt of Central Europe, sedimentary basins locally increase to more than 10 km depth. The upper continental crust is much better exposed for sampiing and investigation than the lower crust. Two comprehensive chemical studies on the composition of the upper crust reported comparable results ( S h a w et al., 1967, 1976, 1986; Taylor and McLennan, 1985). Their results differ distinctly in Be, B, Cu, Zn, Ba, Ta, and Bi. Shaw et al. (1967, 1976) analysed 8,512 rocks from large areas of the Canadian Shield mainly in composite samples. They grouped them into six lithologic varieties. Taylor and M c L e n n a n ( 1985 ) based their minor and trace element data on analyses of shales, loesses, and greywackes in the assumption that the processes of erosion and sedimentation produced an average sample of the exposed crust. They corrected for element fractionation during weathering and sedimentation from REE distribution and element ratios, well k n o w n from isotope geochemistry. Their major element data were adopted from those on the Canadian Shield composition and their data on Zn, Cd, T1, Pb, and Bi Ingerson Lecture 1219 Standard Profile of the Continental Crust (EGT) 62 % Archean - Proterozoic Crust (45.5 km thick) 38 % Proterozoic - Phanerozoic Crust (30 km thick) (Mass of Bulk Cont. Crust: 2.13 x 1019 t) Sediment. Rocks (14 % U. Cr.) o2 D Felsic Intrusives (10.4 km= 50 % Upper Cr.) Gabbros (1.3 km = 6 % Upper Cr.) / Sedimentary Rocks* - - 44.0 % 20.9 % 20.3 % 14.6 % Felsic Intrusives ** 50 40 10 Gabbros (LE MAITRE, 1976) ¢,J Shales, Siltstones (RONOV and YAROSHEVSKIY, 1968) Sandstones, Greywackes ( R and Y, 1968) Mafic etc. Volcanics ( R and Y, 1968) Carbonates (0.8 % Evaporites) ( R and Y, 1968) .... % Granites (WHALEN et al., 1987; LE MAITRE, 1976) % Granodiorites (LE MAITRE, 1976) % Tonalites (this publication) (q cO Gneisses, Mica Schists Amphibolites, Marbles (6.3 km = 30 % Upper Cr.) Metamorphic Rocks *** 64 % (Low- and Medium ......._-~ 15.4 % Grade) "~ 17.8 % 2.6 % Felsic Granulites (61.5 % of Lower Crust) 02 Mafic Granulites (38.5 % o1 Lower Crust) Gneisses (POLDERVAART, 1955) Mica Schist (POLDERVAART, 1955) Amphibolites (POLDERVAART, 1955) Marbles (RONOV and YAROSHEVSKIY, 1968) Felsic Granulites - - (50 % Archean, 50 % Post-Archean) (RUDNICK and PRESPER, 1990) Mafic Granulites - - (RUDNICKand PRESPER, 1990) i< Abundances in 73 % Geosynclines and 27 % Platforms according to RONOV and YAROSHEVSKIY (1968) Abundances according to DALY (1933) and MOORE (1959) Abundances according to RONOV and YAROSHEVSKIY (1968) Abundance of Carbonates reduced from 17.6 to 14.6 % according to Carbon Isotope Balance FIG. 2. Standard profile of the continental crust derived from the 3000 km long European Geotraverse generalized on the basis of worldwide mapping, petrological studies and chemical balances (Table 5 etc.). Table 1 Element concentrations (in ppm) in the Upper Continental Crust (UC) and the Lower Continental Crust (LC) (For references see footnotes in Table 2) UC LC UC/LC UC LC UC/LC UC LC UC/LC Si 303480 271330 1.1 Ce 65.7 53.1 1.2 Yb 1.5 2.5 0.60 A! Fe Ca 77440 30890 29450 82120 57060 48600 0.94 0.54 0.61 Ni Nil La 18.6 25.9 32.3 99 28.1 26.8 0.19 0.92 1.2 U Br Ge 2.5 1.6 1.4 0.93 0.28 (1.4) 2.7 5.7 1.0 Nil Mg K 25670 13510 28650 21200 31550 13140 1.2 0.43 2.2 Cu Co y 14.3 11.6 20.7 37.4 38 27.2 0.38 0.31 0.76 Be Mo Eu 3.1 1.4 0.95 1.7 0.6 1.6 1.8 2.3 0.59 Ti 3117 3240 5010 588 0.62 5.5 Nb 26 22 11.3 13 2.3 1.7 Ta | 1.5 1.4 0.84 0.14 F CI Sr Zr 665 527 953 668 611 640 316 237 872 929 408 568 429 278 352 165 0.75 S¢ 0.57 G a 2.3 Pb 1.2 B 1.4 Th 2.3 P r 0.90 [Sm 1.4 HI" 7 14 17 17 10.3 6.3 4.7 5.8 25.3 17 12.5 5 6.6 7.4 6.0 4.0 0.28 0.82 1.4 3.4 1.6 0.85 0.78 1.5 0.62 1.4 0.50 0.75 0.27 0.31 0.102 0.055 0.99 0.6 0.81 0.26 0.43 0.30 0.101 0.080 0.63 2.3 0.62 2.9 0.63 1.0 1.0 0.69 Cr V Rb Zn N 35 53 110 52 83 228 0.15 149 0.36 41 2.7 79 0.66 34 [2.4 Gd 2.8 2.9 2.5 5.8 2.0 5.4 4.7 2.1 0.8 1.3 0.52 0.62 1.2 7.3 1.5 0.123 0.083 0.061 0.056 0.037 0.170 0.052 0.021 3.3 0.47 1.2 2.7 C p Mn S Ha Li Dy Sn Cs As Ho W Tb T| Lu Sb Cd Ag Bi Se In Hg 1.8 10 K. H. Wedepohl 220 Table 2 Element'concentrations in the Continental Crust (For major elements as oxides see Table 3 and for references see footnotes) O 47.2 %a Nd 27 ppm a Mo 1.1 ppm o Si 28.8 %a Cu 25 ppm a Br 1.0 ppm P 7.96 % a Co 24 ppm a W 1.0 ppm q AI a Fe 4.32 % a Y 24 ppm Ca 3.85 % a Nb 19 ppm a 18 ppm a Sc Na 2.36 % a Mg 2.20 % a K 2.14 % a Ti 4010 ppm C b 1990 ppm P Mn S 757 ppm a a 716 ppm b 697 ppm Ba 584 ppm c F 525 ppm CI 472 ppm d d r 800 ppb Ho 800 ppb a Tb 650 ppb a 16 ppm a TI 520 ppb s Ga 15 ppm a Lu 350 ppba Pb 14.8 ppm a Tm 300 ppb g ppm f Sb 300 ppb t Th 8.5 ppm a Se 120 ppb u Pr 6.7 ppm g Cd 100 ppb s Sm 5.3 ppm a Bi 85 ppb s Hf 4.9 ppm a Ag 70 ppb v Gd 4.0 ppm a In 50 ppbw Dy 3.8 ppm g Hg 40 ppb x Te (5) ppb y Li a I B 11 Sr 333 ppm a Cs 3.4 ppm h Zr 203 ppm a Be 2.4 ppm i Au Cr 126 ppm a Sn 2.3 ppm k Pd 0.4 ppbaa V 98 ppm a Er 2.1 ppm g Pt 0.4 ppb aa Re 0.4 ppb bb 2.5 ppb z Rb 78 ppm a Yb 2.o ppm a Zn 65 ppm a As 1.7 ppm 1 Ru 0A ppb aa N 60 ppm e U 1.7 ppm a Rh 0.06 ppb aa m Ce 60 ppm a Ge 1.4 ppm Ni 56 ppm a Eu 1.3 ppm a 30 ppm a Ta 1.1 ppm n La Os Ir 0.05 ppb bb 0.05 ppb aa UC = Upper Crust, LC = Lower Crust a UC: SHAW et al. (1967, 1976), LC: RUDNICK and PRESPER (1990) in the proportions of Fig 2 b Fig. 7 c UC: calculated from rock averages compiled by PUCHELT (1972) in the proportions of Fig. 2, LC: RUDNIK and PRESPER (1990) d UC: calculated from rock averages complied by WEDEPOHL (1987) in the proportions of Fig. 2, LC: averages of e UC, LC: calculated from rock averages compiled by WLOTZKA (1972) in the proportions of Fig. 2 (additional data on granulites and gabbro granites HALL, 1988) f UC: calculated from rock averages compiled by HARDER (1974) and SHAW et al. (1986) in the proportions of Fig. 2, LC: data from TRUSCOTT et al. (1986), LEEMAN et al. (1992) and HARDER (1974) g interpolated from smooth curve of chondrite normalized REE distribution in the continental crust h UC: Rb/19 acccording to MCDONOUGH et al. (1992), LC: RUDNICK and PRESPER (1990) i UC: calculated from rock averages compiled by HOERMANN (1969) in the proportions of Fig. 2, LC: SIGHINOLFI(1973) k UC: calculated from rock averages compiled by HAMAGUCH~and KURDODA (1969) and SMITH and BURTON (1972) in the proportions of Fig 2, LC: RUDNICK anddd PRESPER (1990) Ingerson Lecture 1221 Table 2. (Continued) 1 UC: calculated from rock averages of ONISH/ and SANDELL (1955), BURWASH and CULBERT (1979) in the proportions of Fig., 2, LC: gabbro, gneiss minus 20% granite m UC: calculated from rock averages compiled by HOERMANN (1970) and ONISHI (1956) in the proportions of Fig. 2, LC: gneiss, gabbro n UC: calculated from Nb/Ta = 17.5 (from international reference rocks) GLADNEY et al. (1983), LC: RUDNICK and PRESPER (1990) o UC: calculated from rock averages compiled by MANHE1M and LANDERGREN (1978) in the proportions of Fig. 2, p UC, LC: calculated from rock averages compiled by FUGE (1974a) (partly corrected with C1/Br ratio 1000) in the q UC, LC: calculated from rock averages compiled by KRAUSKOPF (1970) in the proportions of Fig. 2 gabbro, gneiss minus 20% granite proportions of Fig. 2. Sedimentary rocks calculated with C1/Br = 290 (seawater) r UC: calculated from rock averages compiled by FUGE (1974b) and BECKER et al. (1972) in the proportions of Fig. 2 considering accumulation in C,,~ rich sediments (C/I correlation of PRICE et al. 1970), LC: estimated s t UC, LC: calculated from rock averages ofHEINRICHS et al. (1980) in the proportions of Fig. 2 UC: calculated from rock averages of ONISI-II and SANDELL (1955) and BURWASH and CULBERT (1979) in the proportions of Fig. 2, LC: estimated u UC, LC: calculated from rock averages of KOLJONEN (1973) and KELTSCH (1983) in the proportions of Fig. 2, S/Se in crustal rocks except sediments: 8.5 x 103 v UC, LC: calculated from rock averages of HAMAGUCHI and KURODA, (1959) in the proportions of Fig. 2, Cu/Ag in felsic rocks 300 to 450 w UC, LC: calculated from rock averages compiled by LINN and SCHMITT (1972) and contributed by VOLAND (1969) in the proportions of Fig. 2 x UC, LC: calculated from rock averages compiled by the present author partly from MAROWSKI and WEDEPOHL y UC, LC: order of magnitude estimated from data on international reference rocks (GLADNEY et al., 1983, z UC: calculated from rock averages compiled by CROCKET (1974) in the proportions of Fig. 2, LC partly from (1971) and partly from unpublished data of HEINRICHS in the proportions of Fig 2 SIGHINOLFI et al. 1979) and on MORB (HERTOGEN et al. 1990) SIGHINOLFI and SANTOS (1976) partly from gabbro aa UC, LC: from composite sample of 17 European greywackes analysed by ICP MASS in nickel sulfide extract after Te coprecipitation (HARTMANN, 1995) bb UC: ESSER and TLrREKIAN (1993) f r o m Heinrichs et al. ( 1 9 8 0 ) . T h e y calculated u p p e r crust averages o f Li, Be, B, Ge, As, Se, Zr, M o , Ag, In, Sb, Ba, W , and Re f r o m the r e s p e c t i v e c o m p i l a t i o n s edited by W e d e p o h l ( 1 9 6 9 - 1 9 7 8 ) . T h e f o r m e r authors obtained a granodioritic bulk c o m p o s i t i o n for the u p p e r continental crust. Large sets o f s e d i m e n t a r y rock s a m p l e s f r o m g e o s y n c l i n e s and platforms have b e e n a n a l y s e d by R o n o v and Y a r o s h e v s k i y ( 1 9 6 8 ) to get an a v e r a g e c o m p o s i t i o n o f the s e d i m e n t a r y top o f the crust. This has e s p e c i a l l y a c c u m u l a t e d s o m e rather m o b i l e c o m p o u n d s , partly o f volatile e l e m e n t s ( C a C O 3 , NaC1, e t c ) . A c o m p r e h e n s i v e c o m p i l a t i o n o f c h e m i c a l data on granulites as the m o s t a b u n d a n t l o w e r crustal rocks has b e e n p u b l i s h e d b y R u d n i c k and P r e s p e r ( 1 9 9 0 ) . A distinct d i s c r e p a n c y in estimates about the size and c o m position and in a s s u m p t i o n s about the g e n e s i s o f the l o w e r and the bulk crust exists b e t w e e n the widely used report o f T a y l o r and M c L e n n a n ( 1 9 8 5 ) and the results o f our p r e s e n t investigation. T h e s e authors a s s u m e that the l o w e r crust c o m prises 75% o f the total crust in contrast to our a b o v e listed 50% estimate b a s e d o n the E G T s e i s m i c profile t h r o u g h Europe. T a y l o r and M c L e n n a n ( 1 9 8 5 ) calculated the average l o w e r crust c o m p o s i t i o n by r e m o v a l o f their u p p e r from their bulk crust c o m p o s i t i o n . T h e y got a l o w e r crust w h i c h is distinctly m o r e mafic ( 5 4 . 4 % SIO2) than average diorite or andesite ( 5 7 . 7 % SIO2; Le Maitre, 1976). T h e f o r m e r authors m o d e l l e d a dioritic continental crust f r o m their A r c h e a n crust c o m p o s i t i o n ( 7 5 % ) and f r o m island arc andesites ( 2 5 % ) . Their A r c h e a n crust consists o f a 2:1 mixture o f mafic ( M O R B ) and felsic (tonalitic to t r o n d h j e m i t i c ) e n d m e m b e r s , w h i c h is in R E E c o m p o s i t i o n c o n f o r m a b l e with andesites ( o r d i o r i t e s ) . The m o d e l p r o p o s e d by Taylor and M c L e n n a n ( 1985 ) o b v i o u s l y o v e r e s t i m a t e s the a b u n d a n c e s o f andesites and diorites at active continental m a r g i n s and in the bulk crust. T h e s e authors stated that their m o d e l is constrained by the a s s u m p t i o n o f about 4 0 % o f the total heat flow at the average E a r t h ' s surface b e i n g d e r i v e d f r o m the crust and 60% f r o m the mantle. T h e y have calculated that for the r e s p e c t i v e heat p r o d u c t i o n a bulk crust a b u n d a n c e o f 9000 p p m K, 3.4 p p m Th and 0.9 p p m U is required. I n f o r m a t i o n f r o m refraction seismic profiles on the crustal structure and c o m p o s i t i o n is e x p e c t e d to be m o r e reliable than crustal m o d e l s b a s e d on heat p r o d u c t i o n o f the silicate earth. 1222 K.H. Wedepohl Tonalltes/Continental Greywaekes/Continental Crust Crust 10.0-- --10.0 8.0-- 8.0 6.0-- -- 6.0 4.0 B -- 4.0 3.0 -- 3.0 -- 2.0 m 2.0m AM P Sr,Ga 1.0 4 0.8__ Na Pr,Tb,Yb Ti,A ,Eu,Gd,Lu Si,Fe,Ba,V,Li~Pb,Sn,U,Ta K,Rb,Zr,La,Cu,Th Zr Mn,Ca,Zn,Ce,Nd,Y,Sm,H f,Dy,Er,Cs - Si,Zn,La,Y,Ga,U Ti,Mn,V,Ce,Cu Sc,Pb,Th,Gd,Er,Yb,Ho,Tb,Lu K P,Ba,Cr,(Hf),Cs Mg,Co,Sc Mg,Sr,Co 0.6 m Nb / m 1.0 -- 0.8 -- 0.6 -- 0.4 -- 0.3 Ca Ni,Nb - 0.4 D 0.3 __ AI,Fe,Na,Nd,Pr,Sm,Dy,Eu,Rb Cr, Ni 0.2-- -- 0.1 m -- 0.2 0.1 FIG. 3. Average composition of tonalites and greywackes from worldwide sampling (Table 3) in comparison with the composition of the continental crust. CRUSTAL CONCENTRATIONS OF MAJOR ELEMENTS AND COMMONLY ANALYSED MINOR ELEMENTS We have recalculated the composition of the continental crust in the proportions of upper crust to lower felsic crust to lower mafic crust being equal to about 1:0.6:0.4 as derived from the EGT refraction seismic profile through Europe. The precise proportion of these units and of additional subunits in a standard crustal profile is listed in Fig. 2. The abundance of major sedimentary, magmatic, and metamorphic rocks in the subunits of the continental crust is derived from the evaluation of mapping and drilling reports (mainly from Ronov and Yaroshevskiy, 1968; Daly, 1933; Moore, 1959; supplemented by additional authors). The chemical composition of the upper and the lower continental crust is for the majority of commonly analysed elements taken from Shaw et al. ( 1976, 1986) and from Rudnick and Presper (1990), respectively. The latter authors presented averages of Archean and post-Archean felsic granulites from terrains ( which we used in a proportion of I : 1 ) and of mafic granulites sampled as xenoliths. Our data for the upper and lower continental crust and for the bulk continental crust are presented in Tables 1 and 2, respectively. These tables also contain data on additional elements which were not considered in the above-mentioned references. They will be handled in the next section. Our bulk crust has a tonalitic composition (cf. Fig. 3) and is also close to the average of felsic granulites of Rudnick and Presper (1990) and not much different (except Fe and Ta) from the felsic granulites of Shaw et al. (1986). The continental crust calculated by us (Tables 1 and 2) has about twice the concentration of heat producing elements of the crustal model suggested by Taylor and McLennan ( 1985 ). There exists ample experimental evidence (Rushmer, 1991 ; Wolf and Wyllie, 1991; Springer and Seck, 1995; Rapp, 1994) that tonalites are partial melting products of mafic rocks under water-undersaturated conditions. This suggests that a part of the felsic lower crust has formed from tonalitic partial melts derived from the mafic lower crust after supply of water from mafic intrusions and dehydration of subducted ocean crust. This water might have introduced a certain fraction of K and other incompatible elements into the volume of partial melting. A part of the felsic lower crust is residual from the formation of granitic partial melts during orogenic heating. We have calculated the composition of a felsic lower crust fragment after subtraction of 30% granitic partial melt (1:1 mixture of I- and S-type felsic granites of Whalen et al., 1987). The residuum has a major element composition close to diorites as listed in Table 4. The minor elements Sc, Cr, Co, Ni, and HREEs increased and Rb, Cs, Pb, Th, and U decreased in the residuum relative to the felsic lower crust after granitic melt separation. The minor dioritic residuum stays in the predominantly tonalitic substratum of the felsic lower crust, which preserves its overall tonalitic composition. Greywackes approach on average the chemical composition of tonalites with the exception of B, Zr, Si, Ca, P, and Cr (Table 3, Fig. 3). This characterizes them as major products of erosion at active continental margins and indicates the importance of tonalites as early products of magmatism generating new continental crust at plate boundaries. The average metamorphic rocks of the continental upper crust (64% gneiss, 15% mica schist, 18% amphibolite; cf. Fig. 2) and especially their major proportion of gneisses are close in chemical composition to tonalites and greywackes, the latter Ingerson Lecture with the exception of SiO2. The chemical connection indicates genetic relationship. A critical proof of the representativeness of the Canadian Shield major element data for the composition of the upper continental crust is presented in Table 5. In this table chemical compositions of major subunits of the upper continental crust are summed up with the statistical weight of their abundance as listed in Fig. 2. The sum of the subunits in Column H is compared with the Canadian Shield data of Shaw et al. (1976). There exists a good correspondence between the two sets of data with a little more than 10% deviation in SIO2, TiO2, Fe203, and Na20. The deviation in Na20 decreases but does not disappear if the seawater reservoir of this element is considered. The deviation in SiO2 might be caused by the mobility of this compound in hot water and its accumulation in quartz veins. Some other minor deviations could depend on our choice of data for rock units in Table 5. The good correspondence has encouraged us to use the Canadian Shield as representative of the upper continental crust. It additionally suggests to employ the rock abundances of Fig. 2 as statistical weight for the calculation of minor element abundances not considered in the investigations by Shaw et al. ( 1967, 1976, 1986) in a later section. After a critical proof of the major set of data on the upper crust we have to test the reliability of our assumptions on the bulk crust. For this test we use the experience about the crustal and bulk earth distribution of several radioactive and radiogenic isotopes. Some elements which have important radioactive/radiogenic isotopes are connected by close crystal chemical relations. Rb, Th, U, K, and Pb are highly incompatible in mantle minerals and therefore extremely accumulated in the continental crust relative to the primitive mantle (factor hundred; cf. Fig. 5). Pairs of element abundances in the continental crust, which are neighbors or almost neighbors in the sequence of incompatibility of Fig. 5 form element ratios in which they do not differ much from the respective primitive mantle ( P M ) ratios, the latter as reported by Hofmann (1988). The T h / U ratio is 5 in the calculated crust and 4 in the PM. The more incompatible Th being more enriched in the crust. Asmerom and Jacobsen (1993) have calculated an average T h / U ratio of 4.1 from the lead isotopic composition of suspended river loads with a Nd model age from 0.5-3.5 Ga. This result although conformable with our T h / U ratio of the upper crust (Table 1 ) might suggest a slightly smaller ratio than 5 for the bulk crust. Our K / U ratio is 1.26 × 104 for the bulk crust compared with 1.27 × 104 in the PM. The U / P b and K / P b ratios are 0.115 and 1445 in the crust and 0.116 and 1475 in the PM, respectively. The K / R b ratio is 274 in the crust and 482 in the PM with the less mantle compatible Rb being more enriched in the crust. The R b / S r and U / P b systems important for the crust are interconnected by the K / R b and K / U relations. The crustal behavior of Rb, Pb, T1, and several other elements is controlled by their crystal chemical connection to K and their affinity to the feldspar and mica structures. Minor differences in this behavior between Rb, Pb, and T1 are reflected in the different slopes of element distributions in major rock types plotted in Fig. 6. The link between the R b / S r and S m / N d systems is the comparable mantle incompatibility of Sr and Nd (Fig. 5 ). The 1223 S r / N d ratios for the continental crust and the PM are 12.3 and 15.3 with the slightly more compatible Sr causing the lower crustal ratio. We have used the element or isotope ratios of worldwide river loads to check our calculated bulk crust (Table 2) and upper crust (Table 1 ) element ratios (Fig. 4). Erosion has apparently favoured the upper crust slightly more than the lower crust as reflected in the R b / S r and U / P b systems. In a plot of chondrite normalized REE concentrations the elements with high analytical precision give a smooth curve. We have corrected the REEs with lower analytical precision and have estimated the Pr, Dy, Er, and Tm concentrations, which were not analysed in the Canadian Shield, by interpolation in that curve. The final values are presented in Table 2. Our crustal L u / H f ratio is the same as that reported by Patchett et al. (1984) for common sedimentary rocks (except pelagic deposits) and used for their isotope studies. The check by isotope constraints suggests that the use of the data by Shaw et al. ( 1967, 1976) on the upper crust and those by Rudnick and Presper (1990) on the lower crust in the proportions derived from the EGT profile is recommended for a calculation of the bulk crust composition. CRUSTAL CONCENTRATIONS OF RARELY ANALYSED ELEMENTS Table 2 contains major element and thirty-two minor element data from our investigation in the former section. The gaps in Table 2 to be filled in this section concern thirty-three additional minor elements. For two of them (Ba, Ta) Shaw et al. ( 1967, 1976) and Taylor and McLennan (1985) report very different concentrations ( 1070 and 550 ppm Ba, 5.7 and 2.2 ppm Ta, respectively) for the upper crust. The average Ba concentrations analysed in the Canadian Shield are even different between Shaw et al. ( 1967, 1976) and Eade and Fahrig (1971) (1070 and 810 ppm Ba). If we use the rock abundances listed in Table 2 and Ba averages for common rock species as reported by Puchelt (1972) we get an upper crust value of 668 ppm Ba which is intermediate between the upper crust value of Taylor and McLennan ( 1985 ) and the Canadian Shield concentration of Eade and Fahrig (1971). Our B a / U (344) and B a / T h (68.7) ratios are slightly higher and lower than the respective PM ratios (298, 74.4; Hofmann, 1988), which indicates that either the mantle incompatibility of Ba has to be positioned (in deviation from Fig. 5) between Th and U or that the crustal abundance of Ba could be slightly higher. In every case should the crustal B a / R b ratio be lower than the PM ratio of 11.3. It could be a little higher than our present value of 7.5. If we calculate the Ta concentration in the upper crust from the Nb concentration by the use of the PM ratio of 17.6 (Hofmann, 1988) the value of 1.5 is still slightly lower than 2.2 ppm Ta reported by Taylor and McLennan (1985). Our calculation is supported by the fact that analytically very precise data on seven standard reference rocks (granites, basalts, andesite) compiled by Gladney et al. (1983) have on average a N b / T a ratio of 17.7. Older data on common rocks as those compiled by Wedepohl (1978) give lower N b / T a ratios closer to 10 than to 17.6. This is probably an analytical problem. For two of the rather abundant minor elements (C and S), for which we have not many reliable data on magmatic and 224 K. H. Wedepohl Table 3 Average concentration of elements in tonalites and greywackes from worldwide sampling in comparison with the Continental Crust SiO2 Ti02 A1203 Fe203 MnO A Continental crust B Tonalites 61.5% 0.68 15.1 6.28 61.9 % 69.1% 0.77 0.72 C Greywackes B/A 1.00 1.13 CIA 1.12 1.06 16.3 13.5 1.07 0.89 6.3 5.9 1.00 0.94 o. 10 0.09 0.10 0.90 1.00 MgO 3.7 2.6 2.3 0.70 0.62 CaO 5.5 4.9 2.6 0.89 0.47 Na20 3.2 3.9 3.0 1.22 0.94 K20 P205 Ua Sr Zr 2.4 2.O 0.79 0.83 11.l 8 584 ppm 333 203 0.13 /I.72 Cr 0.70 1.9 0.26 608 ppm 439 173 302 1.44 1.04 1.32 0.85 126 38 88 (I.30 V 98 1113 98 1.(16 1.00 Rb 78 64 72 0.82 0.92 Zn 65 61 76 0.94 1.16 Ce 60 53 58 0.89 0.96 Ni 56 19 24 o.34 0.43 La 30 23 34 0.77 1.13 Nd 27 25 25 0.93 0.93 Cu 25 19 24 0.76 0.98 Co 24 16 15 (1.67 0.63 Y Nb 24 22 26 0.93 1.08 I).46 0.44 Li 18 19 Sc 11 16 0.67 Ga Pb B 16 15 19 16 1.30 1.08 14.8 t4.2 14.2 0.95 0.95 Th 8.5 6.4 9.0 0.76 1.06 Pr Sm Hf Gd 67 8.5 6.1 0.91 5.3 4.9 4.6 4.9 4.6 3.5 4.2 4.0 Dy 4.o 3.8 3.5 3.4 1.27 0.92 0.93 1.05 i0.92 Cs 3.4 3.2 2.2 !/}.93 0.65 Sn 2.3 2.4 Er 2.1 1.9 2.2 Yb 2.0 1.7 2.4 1.7 2.1 2.0 1.3 1.4 1.1 900 ppb 750 370 1.2 U En Ta He Tb Lu An Pd Pt Ru 19 8.8 1.1 650 350 2.5 0.4 0.4 0.1 2111 8.4 0.73 0.60 1.49 1.06 37 11 800 ppb 426 ppm 780 ppb 630 370 4.8 0.4 0.4 0.1 1.011 3.3 1.04 0.90 1.20 1.00 1.06 1.00 I. 11 1.15 1.06 0.86 0.71 1.00 0.911 1.02 1.05 1.16 0.88 0.98 0.96 1.06 Ingerson Lecture 1225 Table 3 (continued) A Continental B Tonalites C Greywackes B/A ( 7A crust Rh 0.06 0.06 Ir 0.05 0.05 Tonalites: Total average of group averages from USA, Canada, Sri Lanka, Greenland, Finland, UK, Portugal, with equal statistical weight: ARTH et aL (1978), ERMANOVICS et al. (1979), TARNEY et al. (1979), SCHERMERHORN (1987 and person, comm.), PARADIS et al. (1988), POHL and EMMERMANN (1991), WEDEPOHL et al. (1991), TEPPER et al. (1993) Gre'~caekes: Total average of group averages from USA, Canada, Australia, India, Sri Lanka, Germany with equal statistical weight: WEBER (1960), ONDRICK and GRIFFITHS (1969), TAYLOR and McLENNAN (1985), POHL and EMMERMANN (1991), WEDEPOHL (composite 17 greywackes, Germany, unpubl.) metamorphic rocks, we have provided a stable isotope balance to improve the bulk crust abundance values (Fig. 7 ) . These elements occur mainly in two valence states (with very different isotopic characteristics) and are highly accumulated in the sedimentary top of the crust. The bulk crust isotope data of the two balances must be close to the most probable values for the mantle. The carbon balances suggest that the proportion of carbonate rocks in the sedimentary column as calculated by Ronov and Yaroshevskiy ( 1 9 6 8 ) , has to be reduced from 17.6 to 14.6%. The sulfur balance suggests a value for the abundance o f SOn in evaporites. This value is very important for an evaluation of the crustal distribution of C1. The high mobility of NaC1, its abundance in c o m m o n sedimentary rocks and the scarcity of data on chlorine in magmatic and metamorphic rocks are some o f the difficulties for the calculation of a reliable value of the CI abundance in the continental crust which we have investigated in detail (Wedepohl, 1987). This element is highly accumulated in the sedimentary top of the crust ( 5 5 % ) whereas F occurs mainly in the magmatic and metamorphic part of the crust where it replaces OH in mineral structures. The other elements which are especially accumulated in the sedimentary cover are I, Br, B, Hg, N, and As which form mobile a n d / o r volatile compounds (Fig. 8). The crustal abundances in Table 2, which were not reported in the former section, are all calculated from literature data (foot-notes in Table 2) on c o m m o n rocks with the statistical weight of the rock abundances in the upper and lower crust respectively (Fig. 2). For some of the elements (Be, Ge, Mo, I, Sb, In, Te, Pt-group, and Re) reliable literature data on c o m m o n rocks, especially on metamorphic rocks, are rather rare. Sample contamination is a serious problem with several of the rare elements (I, Hg, Pt-group, etc.). Knowledge about the crystal chemical behavior of some rare elements allows a separate check on their crustal abundance. In c o m m o n rocks the following element ratios are almost constant: S i / G e and S i / S n - 105, S / S e ~ 1 0 4, A s / S b ~ 6, C I / B r ~ 300 (sedi- Table 4 Balance of residual rocks after 30% partial melting of felsic lower crust A Felsic lower crust [63.1 SiO~ 0.70 TiO~ AI:O3 Fe:03 MnO MgO B Granites fl and S felsic) 73.4 0.27 C Felsic lower crust minus 30% B 58.7 0.88 D Diorites 57.5 0.95 14.86 13.5 15.4 16.7 6.89 2.0 8.9 8.0 0.10 0.04 0.12 0.12 3.60 0.57 4.9 3.7 CaO 4.83 1.50 6.3 6.6 Na20 3.17 3.10 3.9 3.5 K~O 2.11 4.35 1.2 1.8 P20s 0.18 0.10 0.21 0.29 Reference: RUDNICK and PRESPER(1990) WHALEN ~ a1.(1987) LEMAITRE (1976) 1226 K . H . Wedepohl Table 5 Balance of major rock species in the Upper Continental Crust SiO: TiO2 AI:O3 Fe203 MnO MgO CaO Na20 K20 P20s H~0 + CO:~ Reference A B C Sedimentary rocks (propoa.acc. Fig. 2) Granites (I and S felsi¢) Granodiorites 52.4 0.68 13.7 6.4 0.12 3.3 9.0" 1.65 2.14 0.18 73.4 0.27 13.5 2.0 0.04 0.57 1.50 3. I0 4.35 0.10 0.6 66.1 0.54 15.7 4.4 0.08 1.74 3.83 3.75 2.73 0.18 0.8 3.1 D 61.9 (/.77 16.3 6.3 0.10 2.6 4.9 3.9 1.9 0.26 0.7 5.9* RONOVand WHALEN et LEMAITRE YAROSHEVSKIY al. (1987) (1976) (1968) *corrected acc. Fig 7 Sm Nd Lu Hf Sm/Nd 147Sm / 144Nd Lu/Hf 176Lu / 177Hf G Gabbros Metamorphic Rocks (proport. acc. Fig. 2) Upper continental 15 % A, 25% B, 20% crust C, 4% D, (Canad. Shield) 6% E, 30% F 50.1 1.10 15.5 11.5 0.12 7.6 4.58 2.4 0.9 0.24 0.7 63.7 0.74 15.1 5.96 0.10 2.91 3.88 2.87 3.21 0.22 0.5 1.1 POLDERVAART (1955) 64.9 0.52 14.6 4.4 0.07 2.2 4.1 3.5 3.1 0.15 0.8 LEMAITRE (1976) m e n t s e x c l u s i v e l y ) , K / T I -- 4 x l 0 4 (cf. Fig. 6 ) , K / B i - 2.5 × l 0 s, R b / C s = 19 ( e x c e p t feisic l o w e r crust; M c D o n o u g h et al., 1 9 9 2 ) , C u / A g ~ 4 x 10 2 ( e x c e p t m a f i c r o c k s ) , C u / A u ~ 6 x 10 3 ( e x c e p t m a f i c r o c k s ) . T h e s e q u e n c e o f a b u n d a n c e s o f P t - g r o u p e l e m e n t s in p r i m i t i v e u l t r a m a f i c r o c k s is c o n t r o l l e d b y their c o s m i c a b u n d a n c e a n d the o c c u r r e n c e o f sulfides: Pt > R u > P d > Ir ~ O s > R h . U n d e r the r e d o x c o n d i t i o n s in the c r u s t b e i n g d i f f e r e n t f r o m t h o s e o f the P M the s e q u e n c e c h a n g e s to Pd -- Pt > R u > R h ~> O s , Ir. T h e e l e m e n t M o b e i n g a l m o s t as c o m p a t i b l e as Pr is e x p e c t e d to h a v e a c r u s t a l M o / P r ratio c l o s e to that o f the P M (0.23; N e w s o m et al., 1 9 8 6 ) . O u r ratio o f 0 . 1 6 f r o m T a b l e 2 i n d i c a t e s that M o is s l i g h t l y less i n c o m p a t i b l e at partial m e l t i n g in t h e K / Rb = 255 Rb 78 ppm Sr 333 ppm Rb/Sr = 0234 (0 348 UC, 0.116 LC) 87Rb/86Sr=067 E SHAW el al. (1967, 1976) 64.0 0.59 14.7 4.9 0.08 2.4 14.1 2.9/3.1"* 3.1 0.17 1.0 0.80 Fig. 2 ** includingoceans m a n t l e t h a n Pr. T h e correct o r d e r o f m a g n i t u d e c o n f i r m s the base of our calculated Mo abundance. GENETIC IMPLICATIONS T h e e x p l a n a t i o n o f t h e f o r m a t i o n o f the c o n t i n e n t a l c r u s t h a s to p r o c e e d f r o m the fact that it c o n s i s t s m a i n l y o f tonalites a n d to a m i n o r d e g r e e o f granites, g r a n o d i o r i t e s , a n d m a f i c rocks. T h e p r i m a r y m a g m a s for its g e n e s i s w e r e m a f i c partial melts from the upper mantle. The concentrations of highly i n c o m p a t i b l e e l e m e n t s in the c r u s t e x c e e d t h o s e o f the p r i m itive m a n t l e b y a factor o f h u n d r e d (Fig. 5 ) . M O R B m a g m a s as the m o s t a b u n d a n t partial m e l t s f r o m t h e p r e s e n t u p p e r 5.3 ppm 27 ppm 0.35 ppm 4.9 ppm = 0196 (018UC. 021 LC) = 0.119 = 0071 (0046UC, 0 1 0 7 L C ) =0.10 K/U = 1.2x 104 U 1.7 ppm Th 8.5 ppm Pb 14.8 ppm Th / U = 5.0" (41 UC, 7.1 LC) 238U / 204pb ** = t4 = 8.4 (~ Upper Crust 10.9; It Lower Crust 5.3) *An Upper Crust value of 4.1 is suggested by crustal Pb isotope evolution (STACEY and KRAMERS, 1975) and by load of worldwide rivers (ASMIEROM and JACOBSEN, 1993) 87Rb/86Sr = 0.81 87Sr / 86Sr = 0.716 in load of worldwide rivers draining areas with average model age of 2.1 Ga (GOLDSTEIN and JACOBSEN, 1988) **206pb / 204pb + 207pb / 204pb +208pb / 204pb = 73 (ZARTMAN and HAINES, 1988) Sm / N d = 0.19 in load ol worldwide rivers (GOLDSTEIN and JACOBSEN, 1988) Lu / Hf 0.07 in common sedimentary rocks, e~'cept pelagic clays (PATCHETT et al, 1984) i~BSE ~ 8 (BSE = Bulk Silicate Earth) (WHITE, 1993) Resemblance ~aCont.Cr, ~ I~BSE because of high depletion of U and Pb in the Upper Mantle FIG. 4. Average composition of the continental crust in elements with important radioactive and radiogenic isotopes. Comparison with worldwide river loads. Ingerson Lecture ~ I00 o °°o 100 P°b .~ 60 ~ 40 o Nb,Ta Q. N 20 Oo 6O 40 o o Hf Zr o o o 2O o ~a °o ~ 6.0 2 production of the early upper mantle has probably formed the primordial felsic cores of the continents (McCulloch, 1993). At increasing thickness of the continental crust this process of formation of tonalitic partial melts shifted into the marie lower crust and was controlled by water from mafic intrusions and dehydration of subducted ocean crust. A certain thickness of the tonalitic crust and heat advection has allowed its partial melting to form granitic magmas. Melt separation and uprise of felsic magmas from their source was the major process of chemical fractionation within the continental crust. Additional fractionation was caused by weathering and selective water transport of the weathering products to form greywackes, clays, sands, carbonates, and evaporites. Camir6 et al. ( 1 9 9 3 ) have calculated that Archean greywackes from the Canadian Shield are derived from about 65% tonalites/trondhjemites, 30% tholeiitic basalts, and 5% komatiites which is almost identical with the lower crust composition derived by us (Fig. 2). The almost smooth curve of primitive mantle normalized element concentrations of Fig. 5 is based on a certain sequence of increasing compatibility of elements in the structure of c o m m o n mantle minerals. This was derived by H o f m a n n ( 1 9 8 8 ) and Sun et al. ( 1 9 7 9 ) from element behavior at M O R B formation. The smooth part of the curve of Fig. 5 reflects partial melting of upper mantle rocks as the major - 200 m2oo ooo 4.0 10 o o Ti ooo o 6.0 4.0 o 2.0- 2.0 o o i.o- 1.0 o o - 0.6•=- 0.4 - 1227 0.6 -- 0.4 Ba U K Ce Pr Sir HI Ti Gd Dy Y T~n L~ A, Sc Fie li I I I I I I I I II I t I I I I Rb Th Nb La Pb Nd S m Zr Eu Tb Ho Er Y b Na Ca Cu < Ta Increasing Incompatibility of Elements in Mantle Rocks (according to HO F MANN, 1988) ~5 FIG. 5. Average composition of the continental crust in selected elements normalized to the primitive mantle (ace. to Hofmann, 1988). The elements are plotted in the sequence of increasing compatibility. mantle are characterized by a large depletion of these highly incompatible elements which is complimentary to their accumulation in the crust ( H o f m a n n , 1988). Extensive partial melting in a subducted fraction of the early marie crust which was caused by the relatively high heat K/Rb -2 10 K/Pb -3 10 K/TI 1000 --[ 600 - 1000 - - 600 Continental Crust 400 - _ 400 200 - - 200 100 - MORB 100 Continental Crust 60- 60 40 40 Continental Crust 20_ ~-- 20 MORB 10- ppm Rb, Pb, ppb TI 6 I 0.6 I 1 I 2 t ,° 6 I I I 4 6 10 I I 20 40 I I 60 100 I 200 I I 400 600 I 1000 I 2000 FIG. 6. Correlation of K/Rb, K/Pb and K/TI ratios with Rb, Pb and TI concentrations in abundant crustal rocks (data from Heinrichs et al. 1980, MORB data on K, Rb, Pb from Hofmann, 1988). 1228 K.H. Wedepohl Carbon ppm C Sulfur Mass Proportion 513 C %0 * 7.4 % Sediment. R.: Carbonates 16000** ~ 79.7% Reduced Carbon 4000*** J" 26.5 % Felsic Intrusives 360 5.1% 3.2 % Gabbros 220 0.4% 15.9 % Gneisses, Schists, etc. 820 7.0% 28.9 % Felsic Granulites 820 5.6% 18.1% Mafic Granulites 220 2.2% 0 -25 -15 -13 -13 ppm S ~ Sedimentary Rocks: (Excluding Evaporites Including Evaporites 26.5 % Felsic Intrusives 3.2 % Gabbros 15.9 % Gneisses, Schists, etc. 7.4 % % % % % -15) -6.7 +1.4 +0.5 +3.0 953 75.3 % -2.8 350 500 11.1% 13.6 % +3.0 +0.5 Lower Continental Crust 408 24.7 % +1.8 Continental Crust 697 Upper Continental Crust Continental Crust 1990 (4.2xl 016 t C) *** .... 2860 3810 334 780 690 42.3 13.3 3.5 16.2 -6 %o .... 28.9 % Felsic Granulites 18.1% Mafic Granulites ** Mass ~7 Proportion 534 S %. Abundances mainly from HOEFS (1973), SCHWARCZ (1969), VEIZER and HOEFS (1976), JUNGE et al. (1975), HOEFS (1969) Abundance of Sedimentary Carbonates reported by RONOV and YAROSHEVSKIY (1968) reduced from 22500 to 16000 ppm C to adjust the proportion of Carbonate to Reduced Carbon to 4 : 1 RONOV (1958) The Mantle Source is often reported to contain 513 C from -5 to -6 %o (1.44x1016 t S) -1.66 7 Abundances mainly from RONOV el al. (1974), RONOV and YAROSHEVSKIY (1968), KAPLAN et al. (1963), SIEWERS (1974), SCHNEIDER (1978), WEDEPOHL (1987), WEDEPOHL et al. (1991) q~7 Crustal Sulfur must be supplemented by Seawater Sulfur ( 1 . 4 x 1 0 1 5 t S ; 5 3 4 S + 2 0 %o ) to get 834 S + 0.3 %o (Mantle Source, not far from Meteoritic Troilite) FIG. 7. Balances of C and S and their isotopic composition in the continental earth's crust. process of incompatible element accumulation in the crust. A few deviations from this character can be used to identify additional processes partly connected with the formation of tonalites. The large accumulation of Rb, Ba, K (and C s ) in the continental crust indicates that residual K-feldspar, mica ( a n d amphibole) were unimportant at the formation of tonalitic magmas. W e explain the required shift of Nb, Ta, and Ti in Fig. 5 to positions of larger compatibility in the curve of element distribution to balance the depletion as due to the existence of residual rutile at the formation of tonalitic partial melts (Rapp, 1994). The excess of Zr and H f was caused by the temperature dependent extraction of these elements by the tonalitic melts from their mafic source. An average concentration of 200 p p m Z r in the continental crust indicates temperatures of partial melting not far from 850°C. (Watson and Harrison, 1983). The excess of Pb in the continental crust was explained by Peucker-Ehrenbrink et al. ( 1 9 9 4 ) as due to the hydrothermal leaching of the ocean crust and remobilization of leached Pb at the dehydration of subducted ocean crust into continental magma. The formation and chemical fractionation of the continental crust required water. By far the largest amount of crustal water occurs in the oceans (1.4 x 101st) and the second largest fraction in the porous volume of sediments (0.3 x 10~st). The continental crust (excluding the oceans) contains on average about 2% H 2 0 which is mainly accumulated in the upper crust and its sedimentary top. Dehydration of subducted ocean crust and of hydroxide containing minerals in the continental crust is required for partial melting in the mafic and felsic lower crust, respectively. Mantle degassing has formed the atmosphere and the hydrosphere and has controlled weathering at the Earth's surface as well as the accumulation of C, S, CI, N, Ar, B, As, Br, I, Sb, Se, and Hg. The compositions of the upper and lower continental crust are compared in Fig. 8. The elements which form volatile compounds and the highly incompatible elements characterize the upper crust and 3-d elements are specifically accumulated in the lower crust. This fractionation is mainly caused by the uprise of granitic melts and the preferential intrusion of tholeiitic basaltic magmas into the lower crust due to their compressibility (Kushiro, 1982). Both processes are interrelated. The standard crustal profile of Fig. 2 which was derived from the European Geotraverse is converted into a cartoon with symbolized compositions and processes (Fig. 9 ) . Rock species are drawn almost in their correct proportions with felsic rocks in white and mafic rocks in black. By far the largest proportion of felsic rocks has a tonalitic composition. It is formed in the mafic lower crust and intrudes into the upper together with granitic magmas at orogenic events (Pitcher, 1979). Granitic partial melts from a tonalitic or sedimentary source have increased in their proportion of the crustal magmatic production during Earth's history. Crustal temperatures as calculated by C h a p m a n ( 1 9 8 6 ) are listed in the left part of Fig. 9. In our test area of the EGT, the heat flow density increases from the Scandinavian Shield ( 4 0 m W m -2) through Central Europe (60 m W m -2) to the Alpine orogen (<~90 m W m-2; for details of the M o h o temperature see Banda and Cloetingh, 1992). Orogenic heating which is re- Ingerson Lecture 108- I Cs Br 6- B Ta, TI z- u~ Be, Li Pb, F, Zr 1.00.8- Ba, Cd, Sb Ga, Pr, Sm "-. ~ 0.6- Zn, Ca,Ti, Mn Fe 0.4- 0.2- Bi U, Rb, Hg CI, S, Nb, W Th Cu Mg V C0 Sc ~ Hf, As Na, Ce, La, Sn Si, Ge AI, Nd Sr P'Y Ag Dy, Yb, Eu, Ho,Tb, Lu Ni Cr 0.1 I, Br, C, B, Hg, N, CI, S, As accumulated in the Sedimentary Top of the Upper Crust FIG. 8. Comparison of the average composition of the upper with the lower continental crust (Table 1; references in footnotes of Table 2). quired for partial melting within the crust was mainly caused by mafic intrusions. At a heat flow density of 90 m W m 2 the temperature at M o h o depth is more than 1000°C which allows water undersaturated partial melting of mafic rocks. The for- ._o (..) e-. • d. ~ 6 . 8'E =E °C °C 1229 mation of water undersaturated granitic melts from abundant source rocks requires about 800°C ( J o h a n n e s and Holtz, 1990). In the shield areas with their larger thickness and distinctly lower temperatures mafic granulites can be converted into eclogites (Ringwood, 1975). This material with a density higher than that of lherzolite can sink into the mantle if tectonically separated from the lower crust. This process of delamination, which will exclude very dense upper mantle, is required to recycle the major part of the mafic lower crust back into the mantle. The different stages of the mafic lower crust which was formed during Earth's history must have been in total much thicker than the present lowest part of the crust (average 7 km). One single intrusion such as that of the Ivrea area in northern Italy has about 10 k m thickness. A bulk crust with about 30 k m tonalite required 90 to 120 k m mafic source rocks if their degree of partial melting was 25 to 30%. An open-system behavior of the crust, which was caused by a major delamination of eclogite with excess Eu 2+, is indicated by the depletion of Eu 2÷ in the majority of crustal rocks. The lower crust contains on average a surplus of 0.2 ppm Eu 2÷ (based on data reported by Rudnick and Presper, 1990) and the upper crust has a deficit of 0.58 p p m Eu 2+ (based on data compiled by Wedepohl, 1991, and calculated in the rock proportions of Table 5, last c o l u m n ) . This comparison clearly demonstrates the major depletion of Eu e+ in the bulk continental crust. The result agrees with data from a bulk crust section in China ( G a o et al., 1992). "or. ~E °C Sedimentary Rocks km Diagenesis 150 100 60 5 ~= Plutons of Granites GreenschistFacies 310 200 130 10 C~ Plutons of Tonalites 470 300 180 15 590 350 230 20 700 430 270 25 800 470 300 30 880 550 340 35 970 610 370 40 AmphiboliteFacies GranuliteFacies Mafic Intrusions t"~ Vp ~ f ~ ~ 5.9 - 6.5 (km/s) ~. Mica-Schists, Gneisses, Amphibolites (Conrad Discontinuity) o .o Felsic Granulites Felsic Granulites I 6.5 - 7.5 (Residual from Anatexis) (km/s) Mafic Granulites (Residual from Anatexis) Mafic Granulites Moho Discontinuity OJ E E E 45 E o E o E o 50 Spinel Lherzolites and Spinel Harzburgites > 8 (km/s) Heat Flow Density FIG. 9. Cartoon of the standard profile of the continental crust with temperature-depth relations of 3 geotherms calculated by Chapman (1986). 1230 K . H . Wedepohl T h e crustal c o m p o s i t i o n as calculated in this investigation is distinctly m o r e felsic than that m o d e l l e d by Taylor and M c L e n n a n ( 1 9 8 5 ) . T h e a m o u n t o f the m o s t i n c o m p a t i b l e ele m e n t s in the continental crust c a n n o t have b e e n supplied from the primitive c o m p o s i t i o n o f the upper c o n v e c t i n g m a n tle with 670 k m d e p t h exclusively. M o r e than half o f the crustal reservoir o f Cs, Rb, and Ba and half o f that o f Th, U, and K m u s t originate f r o m the l o w e r mantle. T h e separation o f the c o n v e c t i o n cells o f the u p p e r and l o w e r m a n t l e was apparently interrupted during certain e p i s o d e s w h i c h requires future investigations. Our results on the crustal c o m p o s i t i o n have m a i n l y benefitted f r o m recent research on the l o w e r continental crust. 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